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Preliminary results of the seasonal ozone vertical trends at OHP France Maud Pastel, Sophie Godin-Beekmann Latmos CNRS UVSQ, France  NDACC Lidar Working.

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Presentation on theme: "Preliminary results of the seasonal ozone vertical trends at OHP France Maud Pastel, Sophie Godin-Beekmann Latmos CNRS UVSQ, France  NDACC Lidar Working."— Presentation transcript:

1 Preliminary results of the seasonal ozone vertical trends at OHP France Maud Pastel, Sophie Godin-Beekmann Latmos CNRS UVSQ, France  NDACC Lidar Working Group, 4-8 Nov 2013, TMF, California

2 Previous study Nair et al, ACP 2013 R 2 as a function of altitude and month Multiple regression analysis using QBO 10, 30 hpa, NAO, SFX, HF, AOD 550nm (1985 to 2010) Merged profiles: LIDAR v4, MLS, HALOE v19, SAGE II v6, OHP Soundings  Similar trend results obtained between PWLT with turnaround in 1997 and EESC trend models  Ozone recovery visible on vertical profile time series but signal barely significant 2 methods : Piecewise Linear Trend ( PWLT) Equivalent Effective Stratospheric Clorine

3  New Lidar data  New satellites versions  Times series up to 2012 included  Update proxies until 2012 included  Use additionnal proxies  Seasonal analysis Present study (Preliminary)

4 Stratospheric profiles measurements SatellitesVertical resolution ( km) Altitude ( km) AURA MLS ( 2004 – 2012) L2GP-O3_v2.2115 - 45 SAGE II (1986 – 2005) version 7a115 - 45 GOMOS (2002- 2011) version 5118 – 45 ODIN (2001- 2011) version 2.1218 - 44 MIPAS (2005 -2011) version 5R_O3_2201 10 - 44 GOZCARDS (1986 -2012) version 1.01214 - 44  LIDAR data ( new version: v 5.0 ) have been reprocessed from 1985 until now with the same temperature and pression profiles in order to get homogenous data. Data available on the NDACC data base (ames format, soon in HDF)  For each comparaisons with satellites, LIDAR data have been converted into the same vertical resolution GOZCARDS (Global OZone Chemistry And Related trace gas Data records for the Stratosphere) Merged of SAGE II, HALOE, Aura MLS, UARS MLS and ACE-FTS data sets

5 Monthly mean times series ODIN is systematicaly lower than the LIDAR with a important bias from 28 to 40 km Only MIPAS present a positive bias (of 4.6 %) from 35 to 45 km Consistency between SAGE II and GOZCARDS MLS GOMOS ODIN MIPAS GOZCARDS SAGE II LIDAR

6 Data quality (Relative drift in %/yr) GOMOS SAGE II MLS ODIN GOZCARDS Drift generally within ± 0.5%.y-1 in 25 – 40 km range except Aura MLS and MIPAS Long-term measurements stable at OHP latitude band ( non significant drifts except MIPAS) Avg=0.46%/yr Avg= -0.05%/yr Avg=-0.20%/yr Avg=0.69%/yr Avg=0.01%/yr MIPAS Avg=0.12%/yr

7 Anomalies times series % Between 16 to 21 km, all instruments present strong variations except GOZCARDS LIDAR, MLS and GOZCARDS present the smallest variations

8 Spring (MAM) time series anomaly in % LIDAR GOMOS SAGE II MLS ODINGOZCARDS

9 Summer (JJA) time series anomaly in % LIDAR GOMOS SAGE II MLS ODINGOZCARDS

10 Autumn (SON) time series anomaly in % LIDAR GOMOS SAGE II MLS ODINGOZCARDS

11 Winter (DJF) time series anomaly in % LIDAR GOMOS SAGE II MLS ODINGOZCARDS

12 Regression analysis Proxies used from 1985 to 2013 EESC and PWLT Monthly model using multiple proxies (autocorrelation taken into Account) Proxies used: - QBO (30 & 10 hPa) -NAO index -F10.7 cm Solar flux -Heat flux at 100 hPa averaged over 45-75°N -Aerosols optical thickness at 550 nm -Tropopause altitude above OHP Applied on LIDAR and the merged of all the satellites with the lidar QBO NAO Solar flux Aerosols Tropopause Heat flux

13 LIDAR Variability due to model proxies  QBO significant mainly in winter months (easterly phase)  Aerosols: significant at all month and Altitudes  Solar flux: significant in summer in midstratosphere  NAO mainly signifcant in winter  Heat flux and tropopause: significant mainly in lower Stratosphere

14 Regression analysis LIDAR Merged of all the data Strong variations: LIDAR residual above 40 km ( seasonal variation ?) Merged data below 18 km

15 O 3 Variability explained LIDAR Merged of all the data Variability of O3 less explained above 35 km in Spring and Summer Below 20 km, variability more explained with LIDAR data except in October

16 Ozone vertical distribution trends LIDAR Merged of all the data Post turnaround trends Pre- Turnaround trends

17 Spring ozone vertical distribution trends LIDAR Merged of all the data Post turnaround trends Pre- Turnaround trends Pre-turnaround: LIDAR PWLT and EESC significant around 15-20 km

18 Summer ozone vertical distribution trends LIDAR Merged of all the data Post turnaround trends Pre- Turnaround trends Pre-turnaround: LIDAR PWLT and EESC significant around 15-20 km

19 Autumn ozone vertical distribution trends LIDAR Merged of all the data Post turnaround trends Pre- Turnaround trends Both data set: Similar trends with EESC and PWLT for post-turnaround period for both data except below 20 km Pre-turnaround: PWLT and EESC significant: LIDAR: 30-45 km Merged : 24-45 km

20 Winter ozone vertical distribution trends LIDAR Merged of all the data Post turnaround trends Pre- Turnaround trends Similar trends with EESC and PWLT for post-turnaround period for both data Both data: Pre-turnaround: PWLT and EESC significant From 24-45 km

21 Outlook  Introduction of Umkehr and SBUV II in the present study  Used the equivalent latitude in the regression analysis ( might explain the significant pre-turnaround trend during the Winter period Conclusions Evaluation of long-term ozone trend at OHP using multiple regression analysis for the period 1985 – 2013 Significant pre-turnaround trend depending on the season Post-turnaround increase but mainly unsignificant LIDAR, SAGE II, GOZCARDS and MLS present the smallest anomalies for 1985 to 2013 All Satellites anomalies agree well with the lidar, with average biases of less than ± 5%, in the 20–40 km range

22 Thank you for your attention GOZCARDS team ( NSA, Jet Propulsion Laboratory The NASA Langley Research Center (NASA-LaRC) for provinding SAGEII data Dr. Alexandra Laeng at Karlsruher Institut fur Technologie (KIT) for MIPAS data Dr. Joachim URBAN at Chalmers University of Technology (GOTHENBURG) for ODIN data Dr Alain Hauchecorne at LATMOS ( France) for GOMOS data Dr Lucien Froideveaux ( NSA, Jet Propulsion Laboratory) for AURA MLS data. Thanks to for providing the data


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